218 citations · 1.7k across the 45 of their papers we have counts for
45 papers
The GLEAMing of the first supermassive black holes: II. A new sample of high-redshift radio galaxy candidates
J. W. Broderick, G. Drouart, N. Seymour +27
While unobscured and radio-quiet active galactic nuclei are regularly being found at redshifts , their obscured and radio-loud counterparts remain elusive. We build upon our…
Relation of internal attenuation, dust emission, and the size of spiral galaxies. Calibration at low-z and how to use it as a cosmological test at high-z
M. Lopez Corredoira, C. M. Gutierrez
Dust in spiral galaxies produces emission in the far-infrared (FIR) and internal absorption in visible wavelengths. However, the relation of the two amounts is not trivial because…
Collective motion of run-and-tumble particles drives aggregation in one-dimensional systems
C. Miguel Barriuso Gutierrez, Christian Vanhille Campos, Francisco Alarcon Oseguera +3
Active matter deals with systems whose particles consume energy at the individual level in order to move. To unravel features such as the emergence of collective structures several…
The QUIJOTE Experiment: Prospects for CMB B-MODE polarization detection and foregrounds characterization
F. Poidevin, J. A. Rubino-Martin, R. Genova-Santos +47
QUIJOTE (Q-U-I JOint TEnerife) is an experiment designed to achieve CMB B-mode polarization detection and sensitive enough to detect a primordial gravitational-wave component if th…
Analysis of the Amplitude of the Sunyaev-Zel'dovich Effect out to Redshift z=0.8
M. Lopez-Corredoira, C. M. Gutierrez, R. T. Genova-Santos
The interaction of the cosmic microwave background (CMB) with the hot gas in clusters of galaxies, the so-called Sunyaev--Zel'dovich (SZ) effect, is a very useful tool that allows…
Stellar content of extremely red quiescent galaxies at z>2
M. Lopez-Corredoira, A. Vazdekis, C. M. Gutierrez +1
CONTEXT. A set of 20 extremely red galaxies at 2.5<z<3.8 with photometric features of old passive-evolving galaxies without dust, with stellar masses of ~10^{11} M_sun, have colors…